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High resolution CMB power spectrum from the complete ACBAR data set, , , , , , , , , and 8 other author(s). (2008)cite arxiv:0801.1491 Comment: Submitted to ApJ; Changed to apply a WMAP5-based calibration. The cosmological parameter estimation has been updated to include WMAP5.Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck, , , , , , , , , and 192 other author(s). (2014)cite arxiv:1407.5452Comment: 23 pages, 16 figures, submitted to A&A.An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys, , , , , , , , , and 67 other author(s). (2020)cite arxiv:2002.06197Comment: Submitted to ApJ, 16 pages. arXiv admin note: text overlap with arXiv:1408.3161.A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol, , , , , , , , , and 119 other author(s). (2019)cite arxiv:1907.08605Comment: 10 pages, 3 figures, 1 table; to be submitted to PRL; comments welcome.Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol Data, , , , , , , , , and 59 other author(s). (2020)cite arxiv:2012.01709Comment: 27 pages, 14 figures, accompanying software package available at https://cosmicmar.com/CMBLensing.jl.Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds, , , , , , , , , and 186 other author(s). (2015)cite arxiv:1502.04123Comment: 28 pages, 20 figures. Submitted to A&A.Gravitational Lensing of Cosmic Microwave Background Polarization, , , , , , , , , and 61 other author(s). (2013)cite arxiv:1312.6646Comment: 8 pages, 4 figures. The companion paper describes a measurement of polarization lensing in cross-correlation.Planck 2015 results. I. Overview of products and scientific results, , , , , , , , , and 344 other author(s). (2015)BICEP / Keck XIV: Improved constraints on axion-like polarization oscillations in the cosmic microwave background, , , , , , , , , and 83 other author(s). (2021)cite arxiv:2108.03316Comment: 14 pages, 3 figures.Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust, , , , , , , , , and 192 other author(s). (Sep 25, 2014)